One of the nuclides in each of the following pairs is radioactive. Predict which is radioactive and which is stable: (a) \(\frac{92}{44} \mathrm{Ru}\) and ${ }^{102} \mathrm{Ru},(\mathbf{b}){ }_{56}^{138} \mathrm{Ba}\( and \){ }_{56}^{139} \mathrm{Ba},(\mathbf{c})$ tin -109 and tin-120.

Short Answer

Expert verified
The radioactive nuclides are \(\frac{92}{44} \mathrm{Ru}\), \({ }_{56}^{138} \mathrm{Ba}\), and Tin-109, while the stable nuclides are \({ }^{102} \mathrm{Ru}\), \({ }_{56}^{139} \mathrm{Ba}\), and Tin-120. This is based on comparing their neutron-to-proton ratios, as higher ratios generally lead to greater stability for medium-sized nuclei.

Step by step solution

01

Calculate the neutron-to-proton ratios for each pair of nuclides

To calculate the neutron-to-proton ratio, we need to find the number of neutrons in each nuclide and divide it by the number of protons. Protons can be found in the bottom number, while the difference between the top and bottom numbers represents the neutrons. (a) \(\frac{92}{44} \mathrm{Ru}\): Neutrons = 92 - 44 = 48, ratio = \( \frac{48}{44} = 1.09 \) \({ }^{102} \mathrm{Ru}\): Neutrons = 102 - 44 = 58, ratio = \( \frac{58}{44} = 1.32 \) (b) \({ }_{56}^{138} \mathrm{Ba}\): Neutrons = 138 - 56 = 82, ratio = \( \frac{82}{56} = 1.46 \) \({ }_{56}^{139} \mathrm{Ba}\): Neutrons = 139 - 56 = 83, ratio = \( \frac{83}{56} = 1.48 \) (c) Tin-109: Nuclide is \({ }_{50}^{109} \mathrm{Sn}\) Neutrons = 109 - 50 = 59, ratio = \( \frac{59}{50} = 1.18 \) Tin-120: Nuclide is \({ }_{50}^{120} \mathrm{Sn}\) Neutrons = 120 - 50 = 70, ratio = \( \frac{70}{50} = 1.4 \)
02

Predict the stability based on neutron-to-proton ratios

Based on the calculated ratios, we can now predict the stability of the nuclides. Remember that lighter elements with a nuclear ratio close to 1 are stable and as the atomic number increases, stable nuclei have higher neutron-to-proton ratios. (a) \(\frac{92}{44} \mathrm{Ru}\) has a ratio of 1.09 while \({ }^{102} \mathrm{Ru}\) has a ratio of 1.32. Since the atomic number is 44 (medium-sized nucleus), a higher neutron-to-proton ratio will make the nucleus more stable. Therefore, \({ }^{102} \mathrm{Ru}\) is stable and \(\frac{92}{44} \mathrm{Ru}\) is radioactive. (b) \({ }_{56}^{138} \mathrm{Ba}\) has a ratio of 1.46 while \({ }_{56}^{139} \mathrm{Ba}\) has a ratio of 1.48. They both have close ratios, but since the atomic number is 56 (medium-sized nucleus), a slightly higher neutron-to-proton ratio will favor stability. Thus, \({ }_{56}^{139} \mathrm{Ba}\) is stable and \({ }_{56}^{138} \mathrm{Ba}\) is radioactive. (c) Tin-109 (\({ }_{50}^{109} \mathrm{Sn}\)) has a ratio of 1.18 while Tin-120 (\({ }_{50}^{120} \mathrm{Sn}\)) has a ratio of 1.4. Since the atomic number is 50 (medium-sized nucleus), a higher neutron-to-proton ratio will favor stability. Therefore, Tin-120 is stable and Tin-109 is radioactive. In conclusion, the radioactive nuclides are \(\frac{92}{44} \mathrm{Ru}\), \({ }_{56}^{138} \mathrm{Ba}\), and Tin-109, while the stable nuclides are \({ }^{102} \mathrm{Ru}\), \({ }_{56}^{139} \mathrm{Ba}\), and Tin-120.

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Most popular questions from this chapter

It has been suggested that strontium-90 (generated by nuclear testing) deposited in the hot desert will undergo radioactive decay more rapidly because it will be exposed to much higher average temperatures. (a) Is this a reasonable suggestion? (b) Does the process of radioactive decay have an activation energy, like the Arrhenius behavior of many chemical reactions (Section 14.5\() ?\)

The energy from solar radiation falling on Earth is $1.07 \times 10^{16} \mathrm{~kJ} / \mathrm{min} .$ (a) How much loss of mass from the Sun occurs in one day from just the energy falling on Earth? (b) If the energy released in the reaction $$ { }^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{56}^{141} \mathrm{Ba}+{ }_{36}^{92} \mathrm{Kr}+3{ }_{0}^{1} \mathrm{n} $$ \(\left({ }^{235} \mathrm{U}\right.\) nuclear mass, \(234.9935 \mathrm{u} ;{ }^{141} \mathrm{Ba}\) nuclear mass, $140.8833 \mathrm{u} ;{ }^{92} \mathrm{Kr}\( nuclear mass, \)91.9021 \mathrm{u}$ ) is taken as typical of that occurring in a nuclear reactor, what mass of uranium- 235 is required to equal \(0.10 \%\) of the solar energy that falls on Earth in 1.0 day?

A \(65-\mathrm{kg}\) person is accidentally exposed for \(240 \mathrm{~s}\) to \(\mathrm{a}\) 15-mCi source of beta radiation coming from a sample of ${ }^{90}$ Sr. (a) What is the activity of the radiation source in disintegrations per second? In becquerels? (b) Each beta particle has an energy of \(8.75 \times 10^{-14} \mathrm{~J} .\) and \(7.5 \%\) of the radiation is absorbed by the person. Assuming that the absorbed radiation is spread over the person's entire body, calculate the absorbed dose in rads and in grays. \((\mathbf{c})\) If the RBE of the beta particles is \(1.0,\) what is the effective dose in mrem and in sieverts? (d) Is the radiation dose equal to, greater than, or less than that for a typical mammogram \((3 \mathrm{mSv}) ?\)

Write balanced equations for each of the following nuclear reactions: $(\mathbf{a}){ }_{92}^{238} \mathrm{U}(\mathrm{n}, \gamma){ }^{239} \mathrm{U},(\mathbf{b}){ }_{82}^{16} \mathrm{O}(\mathrm{p}, \alpha){ }^{13} \mathrm{~N},\( (c) \){ }_{8}^{18} \mathrm{O}\left(\mathrm{n}, \beta^{-}\right){ }^{19} \mathrm{~F}$.

The thermite reaction, $\mathrm{Fe}_{2} \mathrm{O}_{3}(s)+2 \mathrm{Al}(s) \longrightarrow 2 \mathrm{Fe}(s)+$ $\mathrm{Al}_{2} \mathrm{O}_{3}(s), \Delta H^{\circ}=-851.5 \mathrm{~kJ} / \mathrm{mol}$, is one of the most exothermic reactions known. Because the heat released is sufficient to melt the iron product, the reaction is used to weld metal under the ocean. How much heat is released per mole of $\mathrm{Al}_{2} \mathrm{O}_{3}$ produced? How does this amount of thermal energy compare with the energy released when 2 mol of protons and 2 mol of neutrons combine to form 1 mol of alpha particles?

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